The origin of unusually hot stars in a sparse cluster has been attributed to their being members of binary systems rather than stellar collisions. This prompts a rethink of how stars merge when they collide. See Letter p.356
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References
Geller, A. M. & Mathieu, R. D. Nature 478, 356–359 (2011).
Burbidge, E. M. & Sandage, A. Astrophys. J. 128, 174–184 (1958).
McCrea, W. H. Mon. Not. R. Astron. Soc. 128, 147–155 (1964).
Hills, J. G. & Day, C. A. Astrophys. Lett. 17, 87–93 (1976).
Hurley, J. R., Pols, O. R., Aarseth, S. J. & Tout, C. A. Mon. Not. R. Astron. Soc. 363, 293–314 (2005).
Mathieu, R. D. & Geller, A. M. Nature 462, 1032–1035 (2009).
Glebbeek, E., Gaburov, E., de Mink, S. E., Pols, O. R. & Portegies Zwart, S. F. Astron. Astrophys. 497, 255–264 (2009).
Stetson, P. B., McClure, R. D. & VandenBerg, D. A. Publ. Astron. Soc. Pacif. 116, 1012–1030 (2004).
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Tout, C. Stars acquire youth through duplicity. Nature 478, 331–332 (2011). https://doi.org/10.1038/478331a
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DOI: https://doi.org/10.1038/478331a